Modeling The X-ray Spectra of the SS 433 Jets

Details Modeling The X-ray Spectra of the SS 433 Jets Modeling The X-ray Spectra of the SS 433 Jets

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.1308m&link_type=abstract

American Astronomical Society, HEAD meeting #10, #13.08

Astronomy and Astrophysics

Astrophysics

Scientific paper

We fit Chandra HETGS spectra obtained for the unusual double-jet X-ray binary SS 433. The emission measure distribution derived from the spectrum can be used to test jet cooling models. New models of the differential emission measure distribution are developed within ISIS and fit to the data.
Support for this work was provided by the National Aeronautics and Space Administration through the Smithsonian Astrophysical Observatory contract SV3-73016 to MIT for Support of the Chandra X-Ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060.

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